Science goals

In the first phase, 5 radio antennas work in a self-trigger array and we try to better understand the challenges in a self-trigger setup in order to capture radio signals from a cosmic ray candidate event.

In the next phase, few particle detectors will be added to the array to work as an external trigger which will increase the accuracy of the results and provides a hybrid detection of cosmic rays.

Few more radio antennas and the required electronics will also be added to the array to increase the overall detection area and the possibility of detecting lower energies cosmic rays considering the threshold of SURA experiment.

Science goals - First Phase

Why Self-trigger?

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